The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder

The Australian SKA Pathfinder (ASKAP) telescope has started to localize fast radio bursts (FRBs) to arcsecond accuracy from the detection of a single pulse, allowing their host galaxies to be reliably identified. We discuss the global properties of the host galaxies of the first four FRBs localized...

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Main Authors: Bhandari, S., Sadler, E.M., Prochaska, J.X., Simha, S., Ryder, S.D., Marnoch, L., Bannister, K.W., Macquart, Jean-Pierre, Flynn, C., Shannon, Ryan, Tejos, N., Corro-Guerra, F., Day, C.K., Deller, A.T., Ekers, Ron, Lopez, S., Mahony, E.K., Nuñez, C., Phillips, C.
Format: Journal Article
Language:English
Published: IOP PUBLISHING LTD 2020
Subjects:
Online Access:http://purl.org/au-research/grants/arc/DP180100857
http://hdl.handle.net/20.500.11937/90940
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author Bhandari, S.
Sadler, E.M.
Prochaska, J.X.
Simha, S.
Ryder, S.D.
Marnoch, L.
Bannister, K.W.
Macquart, Jean-Pierre
Flynn, C.
Shannon, Ryan
Tejos, N.
Corro-Guerra, F.
Day, C.K.
Deller, A.T.
Ekers, Ron
Lopez, S.
Mahony, E.K.
Nuñez, C.
Phillips, C.
author_facet Bhandari, S.
Sadler, E.M.
Prochaska, J.X.
Simha, S.
Ryder, S.D.
Marnoch, L.
Bannister, K.W.
Macquart, Jean-Pierre
Flynn, C.
Shannon, Ryan
Tejos, N.
Corro-Guerra, F.
Day, C.K.
Deller, A.T.
Ekers, Ron
Lopez, S.
Mahony, E.K.
Nuñez, C.
Phillips, C.
author_sort Bhandari, S.
building Curtin Institutional Repository
collection Online Access
description The Australian SKA Pathfinder (ASKAP) telescope has started to localize fast radio bursts (FRBs) to arcsecond accuracy from the detection of a single pulse, allowing their host galaxies to be reliably identified. We discuss the global properties of the host galaxies of the first four FRBs localized by ASKAP, which lie in the redshift range 0.11 < z < 0.48. All four are massive galaxies (log(M ∗/Mo&dot;) ∼ 9.4-10.4) with modest star formation rates of up to 2 M o&dot; yr-1 - very different to the host galaxy of the first repeating FRB 121102, which is a dwarf galaxy with a high specific star formation rate. The FRBs localized by ASKAP typically lie in the outskirts of their host galaxies, which appears to rule out FRB progenitor models that invoke active galactic nuclei or free-floating cosmic strings. The stellar population seen in these host galaxies also disfavors models in which all FRBs arise from young magnetars produced by superluminous supernovae, as proposed for the progenitor of FRB 121102. A range of other progenitor models (including compact-object mergers and magnetars arising from normal core-collapse supernovae) remain plausible.
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spelling curtin-20.500.11937-909402023-05-05T05:46:08Z The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder Bhandari, S. Sadler, E.M. Prochaska, J.X. Simha, S. Ryder, S.D. Marnoch, L. Bannister, K.W. Macquart, Jean-Pierre Flynn, C. Shannon, Ryan Tejos, N. Corro-Guerra, F. Day, C.K. Deller, A.T. Ekers, Ron Lopez, S. Mahony, E.K. Nuñez, C. Phillips, C. Science & Technology Physical Sciences Astronomy & Astrophysics Galaxies Radio continuum emission Radio bursts Star formation GAMMA-RAY BURSTS POPULATION astro-ph.GA astro-ph.GA astro-ph.HE The Australian SKA Pathfinder (ASKAP) telescope has started to localize fast radio bursts (FRBs) to arcsecond accuracy from the detection of a single pulse, allowing their host galaxies to be reliably identified. We discuss the global properties of the host galaxies of the first four FRBs localized by ASKAP, which lie in the redshift range 0.11 < z < 0.48. All four are massive galaxies (log(M ∗/Mo&dot;) ∼ 9.4-10.4) with modest star formation rates of up to 2 M o&dot; yr-1 - very different to the host galaxy of the first repeating FRB 121102, which is a dwarf galaxy with a high specific star formation rate. The FRBs localized by ASKAP typically lie in the outskirts of their host galaxies, which appears to rule out FRB progenitor models that invoke active galactic nuclei or free-floating cosmic strings. The stellar population seen in these host galaxies also disfavors models in which all FRBs arise from young magnetars produced by superluminous supernovae, as proposed for the progenitor of FRB 121102. A range of other progenitor models (including compact-object mergers and magnetars arising from normal core-collapse supernovae) remain plausible. 2020 Journal Article http://hdl.handle.net/20.500.11937/90940 10.3847/2041-8213/ab672e English http://purl.org/au-research/grants/arc/DP180100857 IOP PUBLISHING LTD unknown
spellingShingle Science & Technology
Physical Sciences
Astronomy & Astrophysics
Galaxies
Radio continuum emission
Radio bursts
Star formation
GAMMA-RAY BURSTS
POPULATION
astro-ph.GA
astro-ph.GA
astro-ph.HE
Bhandari, S.
Sadler, E.M.
Prochaska, J.X.
Simha, S.
Ryder, S.D.
Marnoch, L.
Bannister, K.W.
Macquart, Jean-Pierre
Flynn, C.
Shannon, Ryan
Tejos, N.
Corro-Guerra, F.
Day, C.K.
Deller, A.T.
Ekers, Ron
Lopez, S.
Mahony, E.K.
Nuñez, C.
Phillips, C.
The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder
title The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder
title_full The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder
title_fullStr The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder
title_full_unstemmed The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder
title_short The Host Galaxies and Progenitors of Fast Radio Bursts Localized with the Australian Square Kilometre Array Pathfinder
title_sort host galaxies and progenitors of fast radio bursts localized with the australian square kilometre array pathfinder
topic Science & Technology
Physical Sciences
Astronomy & Astrophysics
Galaxies
Radio continuum emission
Radio bursts
Star formation
GAMMA-RAY BURSTS
POPULATION
astro-ph.GA
astro-ph.GA
astro-ph.HE
url http://purl.org/au-research/grants/arc/DP180100857
http://hdl.handle.net/20.500.11937/90940